activity
19942024
most citedA diversity of dusty AGN tori: Data release for the VLTI/MIDI AGN Large Program and first results for 23 galaxies

256 citations · 4.4k across the 147 of their papers we have counts for

collaborators

148 papers

astro-ph.SR2024★ 10 cited

Imaging the innermost circumstellar environment of the red supergiant WOH G64 in the Large Magellanic Cloud

K. Ohnaka, K. -H. Hofmann, G. Weigelt +3

Significant mass loss in the red supergiant (RSG) phase has great influence on the evolution of massive stars and their final fate as supernovae. We present near-infrared interfero…

astro-ph.SR2024★ 6 cited

Contemporaneous high-angular-resolution imaging of the AGB star W Hya in vibrationally excited H2O lines and visible polarized light with ALMA and VLT/SPHERE-ZIMPOL

K. Ohnaka, K. T. Wong, G. Weigelt +1

We present contemporaneous high-angular-resolution millimeter imaging and visible polarimetric imaging of the nearby asymptotic giant branch (AGB) star W Hya to better understand t…

astro-ph.SR2024★ 6 cited

An impressionist view of V Hydrae. When MATISSE paints Asymmetric Giant Blobs

L. Planquart, C. Paladini, A. Jorissen +29

Our purpose is to study the effect of binary companions located within the first 10 stellar radii from the primary AGB star. In this work, we target the mass-losing carbon star V H…

astro-ph.SR2024

Spatially resolving the AGB star V3 in the metal-poor globular cluster 47 Tuc with VLTI/GRAVITY

Keiichi Ohnaka, Gerd Weigelt, Karl-Heinz Hofmann +1

Mass loss at the asymptotic giant branch (AGB) plays an important role not only in the final fates of stars, but also in the chemical evolution of galaxies. Nevertheless, the metal…

astro-ph.SR2024★ 10 cited

Images of Betelgeuse with VLTI/MATISSE across the Great Dimming

J. Drevon, F. Millour, P. Cruzalèbes +31

From Nov. 2019 to May 2020, the red supergiant star Betelgeuse experienced an unprecedented drop of brightness in the visible domain called the great dimming event. Large atmospher…

astro-ph.SR2024★ 10 cited

Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432

J. Varga, L. B. F. M. Waters, M. Hogerheijde +40

Context. Rocky planets form by the concentration of solid particles in the inner few au regions of planet-forming disks. Their chemical composition reflects the materials in the di…